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27 April 2024 |
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Investigation of muon flux anisotropy during CME | | I.I. Astapov
; N.S. Barbashina
; V.V. Borog
; I.S. Veselovsky
; N.V. Osetrova
; A.A. Petrukhin
; V.V. Shutenko
; | | Date: |
31 Dec 2016 | | Abstract: | According to CACTus catalog, during periods of a high solar activity every
day up to tens of coronal mass ejections are observed. Such ejections have an
impact on the flux of cosmic rays that permeate the space around us. Unlike
most ground cosmic ray detectors, muon hodoscope URAGAN (MEPhI) allows to
investigate not only the integrated counting rate of registered particles, but
also the spatial and angular characteristics of the muon flux at ground level.
This approach to particle detection allows fixing changes in the flux of cosmic
rays not only for geoeffective CMEs, but also for the ejections, the front of
which is directed to the opposite side of the Sun. The results of the study of
different types of CMEs at different stages of the solar activity from 2008 to
2015 are presented. | | Source: | arXiv, 1701.0070 | | Services: | Forum | Review | PDF | Favorites | |
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